Mars


Mars is the fourth planet from the Sun and the second-smallest planet in the Solar System, larger only than Mercury. In the English language, Mars is named for the Roman god of war. Mars is a terrestrial planet with a thin atmosphere and has a crust primarily composed of elements similar to Earth's crust, as well as a core made of iron and nickel. Mars has surface features such as impact craters, valleys, dunes, and polar ice caps. Mars has two small, irregularly shaped moons, Phobos and Deimos.

Some of the most notable surface features on Mars include Olympus Mons, the largest volcano and highest-known mountain in the Solar System, and Valles Marineris, one of the largest canyons in the Solar System. The Borealis basin in the Northern Hemisphere covers approximately 40% of the planet and may be a large impact feature.[21] Days and seasons on Mars are comparable to those of Earth, as the planets have a similar rotation period and tilt of the rotational axis relative to the ecliptic plane. Liquid water on the surface of Mars cannot exist due to low atmospheric pressure, which is less than 1% of the atmospheric pressure on Earth.[22][23] Both of Mars's polar ice caps appear to be made largely of water.[24][25] In the distant past, Mars was likely wetter, and thus possibly more suited for life. It is not known whether life has ever existed on Mars.

Mars has been explored by several uncrewed spacecraft, beginning with Mariner 4 in 1965. NASA's Viking 1 lander transmitted the first images from the Martian surface in 1976. Two countries have successfully deployed rovers on Mars, the United States first doing so with Sojourner in 1997 and China with Zhurong in 2021.[26] There are also planned future missions to Mars, such as a NASA-ESA Mars Sample Return set to happen in 2026, and the Rosalind Franklin rover mission, which was intended to launch in 2018 but was delayed to 2024 at the earliest, with a more likely launch date at 2028.

Mars can be viewed from Earth with the naked eye, as can its reddish coloring. This appearance, due to the iron oxide prevalent on its surface, has led to Mars often being called the Red Planet.[27][28] It is among the brightest objects in Earth's sky, with an apparent magnitude that reaches −2.94, comparable to that of Jupiter and surpassed only by Venus, the Moon and the Sun.[16] Mars has been observed since ancient times. Over the millennia has been featured in culture and the arts in ways that have reflected humanity's growing knowledge of it.

The history of observations of Mars is marked by the oppositions of Mars when the planet is closest to Earth and hence is most easily visible, which occur every couple of years. Even more notable are the perihelic oppositions of Mars, which are distinguished because Mars is close to perihelion, making it even closer to Earth.[29]


Animation (00:40) showing major features of Mars
Video (01:28) showing how three NASA orbiters mapped the gravity field of Mars
Geologic map of Mars (USGS, 2014)[70]
Curiosity's view of Martian soil and boulders after crossing the "Dingo Gap" sand dune
Martian plain covered by water ice, precipitated through adhering to dry ice, observed by Viking 2 lander
Proportion of water ice present in the upper meter of the Martian surface for lower (top) and higher (bottom) latitudes
North polar early summer water ice cap (1999); a seasonal layer of carbon dioxide ice forms in winter and disappears in summer.
South polar midsummer ice cap (2000); the south cap has a permanent carbon dioxide ice cap covered with water ice.[115]
A cross-section of underground water ice is exposed at the steep slope that appears bright blue in this enhanced-color view from the MRO.
A MOLA-based topographic map showing highlands (red and orange) dominating the Southern Hemisphere of Mars, lowlands (blue) the northern. Volcanic plateaus delimit regions of the northern plains, whereas the highlands are punctuated by several large impact basins.
Terminology of Martian geological features
Viking 1 image of Olympus Mons. The volcano and related terrain are approximately 550 km (340 mi) across.
Valles Marineris, taken by the Viking 1 probe
Edge-on view of Mars atmosphere by Viking 1 probe
Escaping atmosphere on Mars (carbon, oxygen, and hydrogen) by MAVEN in UV[200]
Detail of a Marsian dust storm, as viewed from orbit
Mars without a dust storm in June 2001 (on left) and with a global dust storm in July 2001 (on right), as seen by Mars Global Surveyor
Dust storms on Mars
18 November 2012
25 November 2012
6 June 2018[214]
29 September 2022
Locations of the Opportunity and Curiosity rovers are noted
Orbit of Mars and other Inner Solar System planets
Curiosity rover’s robotic arm showing drill in place, February 2013
Scoop of Mars soil by Curiosity, October 2012
Enhanced-color HiRISE image of Phobos, showing a series of mostly parallel grooves and crater chains, with Stickney crater at right
Enhanced-color HiRISE image of Deimos (not to scale), showing its smooth blanket of regolith
Ingenuity helicopter on Mars, preparing for its first flight, April 2021
Phobos transits the Sun, as viewed by the Perseverance rover on 2 April 2022
Mars seen through an 16-inch amateur telescope, at 2020 opposition
The War of the Worlds by H. G. Wells, 1897, depicts an invasion of Earth by fictional Martians.